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A Theory for the Maximum Magnitude versus Rate of Decline Relation of Classical Novae

  • Authors: Izumi Hachisu, Hideyuki Saio, Mariko Kato, Martin Henze, and Allen W. Shafter

2020 The Astrophysical Journal 902 91.

  • Provider: AAS Journals

Caption: Figure 9.

Same as Figure 5 but for the chemical composition of Ne2. Each scaling mass (magenta lines) corresponds to the WD mass (from right to left, 0.7–﹩1.35\,{M}_{\odot }﹩ by ﹩0.05\,{M}_{\odot }﹩ steps, except ﹩1.33\,{M}_{\odot }﹩), the same as those tabulated in Table 2 (Ne2). The thick magenta lines of equi-Msc (or equi-MWD) correspond to the WD mass region for neon novae (﹩{M}_{\mathrm{WD}}\geqslant 1.05\,{M}_{\odot }﹩).

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